Rodinia broke up in the first period of the Neoproterozoic, the Tonian. Later its continental fragments were re-assembled to form Pangaea 300–250 million years ago. In contrast with Pangaea, little is known yet about the exact position and history of Rodinia.
The extreme cooling of the global climate around 700 million years ago (the so called Snowball Earth of the Cryogenian period) and the rapid evolution of primitive life during the following Ediacaran and Cambrian periods may have been triggered by the breaking up of Rodinia.
The break-up of Rodinia is better understood than its formation. Extensive flood basalt flows and volcanic eruptions of Neoproterozoic age are found on most continents. This is evidence for large scale rifting about 750 million years ago. As early as 850 and 800 million years ago, a rift developed, eventually becoming an ocean in the Ediacaran.
In a separate rifting event about 610 million years ago (halfway in the Ediacaran period), the Iapetus Ocean formed. It might be that all continental mass was again joined in one supercontinent between roughly 600 and 550 million years ago. This hypothetical supercontinent is called Pannotia.
Its effect on life
Unlike later supercontinents, Rodinia itself was entirely barren. It existed before life colonized dry land. It was before the formation of the ozone layer, so it was too exposed to the ultraviolet radiation in sunlight for any organism (except perhaps bacteria) to live on it. However, its existence probably did affect the marine life of its time.
In the Cryogenian period the Earth experienced large glaciations, and temperatures were at least as cool as today. Substantial areas of Rodinia may have been covered by glaciers or the southern polar ice cap.
The eventual rifting of the continents created new oceans, and seafloor spreading, which produces warmer, less-dense oceanic lithosphere. Due to its lower density, hot oceanic lithosphere does not lie so deep as old, cool oceanic lithosphere. In periods with relatively large areas of new lithosphere, the ocean floors come up, causing the sea level to rise. The result was a greater number of shallower seas.
The increased evaporation from the larger water area of the oceans may have increased rainfall, which, in turn, increased the weathering of exposed rock. This increased rainfall may have reduced greenhouse gas levels. When CO2 level dropped, the period known as Snowball Earth began. Increased volcanic activity also introduced nutrients into the seas. This may have played an important role in the development of the earliest animals.
- Li Z.X. et al 2008. Assembly, configuration, and break-up history of Rodinia: a synthesis. Precambrian Research 160: 179–210
- Zhao, Guochun et al (2002). "Review of global 2.1–1.8 Ga orogens: implications for a pre-Rodinia supercontinent". Earth-Science Reviews 59: 125–162. doi:10.1016/S0012-8252(02)00073-9.
- Zhao, Guochun et al (2004). "A Paleo-Mesoproterozoic supercontinent: assembly, growth and breakup". Earth-Science Reviews 67: 91–123. doi:10.1016/j.earscirev.2004.02.003.
- Template:Cite book chapter: The Rifting of Rodinia
- Template:Cite book
- Donnadieu, Y. et al (2004). "A 'snowball Earth' climate triggered by continental break-up through changes in runoff". Nature 428 (6980): 303–306. doi:10.1038/nature02408. PMID 15029192.